Rosetta makes its reappearance at just the right time for me. The spacecraft, making its second Earth swing-by on November 13, will use its gravity assists past Earth and Mars to reach Comet 67P/Churyumov-Gerasimenko in 2014, deploying a lander onto the nucleus and spending two years orbiting the comet. The close approach produced the memorable image below. I thought I was too under the weather today to post anything, but Rosetta's composite shot of Earth by night offers a short, memorable subject. Look at those city lights! Image: This is a composite of four images combined to show the illuminated crescent of Earth and the cities of the northern hemisphere. The images were acquired with the OSIRIS Wide Angle Camera during Rosetta's second Earth swing-by on Nov. 13. This image showing islands of light created by human habitation was taken with the OSIRIS WAC at 19:45 CET, about 2 hours before the closest approach of the spacecraft to Earth. At the time, Rosetta was about 80,000 km...
Reflections on Space Policy in Washington
About the only thing that went wrong on my Washington DC trip (noted earlier here) was having to fight a persistent head cold and trying to avoid shaking hands with our eminent panelists so as not to contaminate them (I want these guys healthy, and working!). But the fates smiled Wednesday morning when I moderated "The Future of the Vision for Space Exploration," my voice back from what had been near-laryngitis the evening before, and we had a fascinating discussion in the Rayburn House Office Building on Capitol Hill talking about where space exploration is going and what policy decisions loom large at the moment. Louis Friedman, executive director of The Planetary Society, presented a look at current projects to explore the Solar System, many of which are somewhat off our radar, including Indian lunar missions like Chandrayaan-1 and the Chinese lunar orbiter Chang'e I (images expected by the end of this month). Japan's space activities beyond the ongoing Hayabusa asteroid return...
The Milky Way as a Garden
By Larry Klaes Tau Zero journalist Larry Klaes looks at Jon Lomberg's stunning Galaxy Garden in Hawaii. Lomberg told Larry that working on the garden had made him appreciate on a primal level just how many objects there are in even a 'small' section of the Milky Way. So there's one answer to the Fermi Paradox: If extraterrestrial civilizations are out there, maybe they're simply too busy exploring to have gotten around to us! There is a galaxy on Hawaii. Not an actual galaxy, of course, as a typical island of stars contains many billions of suns and spans hundreds of thousands of light years. The galaxy residing on the largest of that particular chain of Pacific islands is a 100-foot wide living representation of the vast stellar realm our planet and humanity dwells in, the Milky Way. Called the Galaxy Garden, the idea for this unique project began about eight years ago in the mind of artist Jon Lomberg, who worked with Cornell University astronomer Carl Sagan on his Cosmos PBS...
On the Road: Space Policy in DC
"The Future of the Vision for Space Exploration" is the title of a panel I'll be moderating tomorrow in Washington DC. In fact, by the time you read this, I should be in transit and looking forward to renewing several good friendships. It's the first session of the Seed/Schering-Plough Science + Society breakfast series, taking place in the House Energy and Commerce Committee Room on Capitol Hill, the goal being to discuss our future in space for an audience of policymakers and Congressional staffers. The event's organizers have lined up quite a panel: Louis Friedman, executive director of The Planetary Society and long-term advocate of a sound and far-reaching space policy, with extensive background at JPL and experience on missions ranging from Mariner to Voyager and Galileo. Steven Squyres, principal investigator for the science payload on the Mars Exploration Rover project, co-investigator on several other Mars missions including the 2009 Mars Science Laboratory, and member of...
The Origin of High-Energy Cosmic Rays?
We have much to learn about cosmic rays but the basics seem established. They are protons and subatomic particles including the nuclei of atoms like hydrogen, oxygen, carbon, nitrogen or iron. Low-energy cosmic rays are known to come from the Sun and presumably other stars, while medium-energy cosmic rays can be explained through stellar explosions. But there are events so powerful that they dwarf all others. A cosmic ray with an energy of 300 billion billion electron volts was detected in 1991, the highest levels ever associated with the phenomena. Where do such ultra-high energy particles come from? They're 100 million times more energetic than anything we can produce with particle accelerators. Fortunately, the fact that they travel more or less in a straight line, not being deflected as strongly as their lower-energy cousins, makes observations of their origin possible. Now the more than 370 scientists working with the Pierre Auger Observatory in Argentina think they have found...
Notes & Queries 11/10/07
When we think interstellar, the possibility of a sudden breakthrough offering quick travel -- Epsilon Eridani in an afternoon -- often dominates the debate. But the second path to the stars is the more gradual migration approach that Gregory Matloff, Les Johnson and the artist C Bangs talk about in their Living Off the Land in Space (New York: Copernicus, 2007). As discussed in this article in the Brooklyn Daily Eagle, the trio made their case at NYC College of Technology/CUNY on Thursday evening, leading off not with a starship but a prairie schooner. The point is trenchant: How can we leverage and extend existing technologies to get us into deep space without breakthroughs in physics? "In going into space, we need to think differently. All of these technologies we describe in our book could be done today," says Johnson (NASA MSFC), who manages the agency's Space Science Programs and Projects Office. Technologies such as solar sails, their great historical precedent being the...
The Sun and its Stellar Twins
If you're looking for an analog to the Sun, you have to do more than find a solitary G-class star. Three stars markedly like the Sun -- 18 Scorpius, HD 98618, and HIP 100963 -- still differ in having several times more lithium than our star. Figuring out whether the low amount of lithium is an unusual trait has ramifications for the search for life in the cosmos. You could theoretically push the issue by saying that the Sun's composition is unlikely to be found elsewhere, making extraterrestrial life rare. But that conjecture, which was a stretch to begin with, may be dampened by the recent findings about HIP 56948. 200 light years away in the constellation Draco, the star mimics the Sun's lithium levels. And there's an additional bonus: Bill Cochran's team, also at McDonald, has demonstrated that HIP 56948 hosts no 'hot Jupiters,' giant worlds so close to their primary that they orbit in a matter of days. Thus this finding, developed using data from the 2.7-meter instrument at...
28th Carnival of Space Online
Emily Lakdawalla is hosting the 28th Carnival of Space at her Planetary Society weblog, a compilation including plenty of coverage on Comet Holmes, the unusually active object that, New Scientist opines, may have suffered a collision with an asteroid. Intriguing speculation, though Centauri Dreams readers will probably find Music of the Spheres' entry on 55 Cancri the most interstellar-minded. Bruce looks at the similarities between that system's new planet and Allen Steele's Coyote. From the novel of the same name, it's a moon orbiting a giant planet in its star's habitable zone, a scenario tantalizingly similar to the recent discovery.
Collecting Natural Antimatter
Robert Forward used to talk about antimatter factories in space, installations that would draw their power from the Sun. He would point out that at a distance of 1 AU, our star delivers a gigawatt of energy for each square kilometer of collector. And being Robert Forward, he thought big: Build a collector array one hundred kilometers on a side to produce a power input of ten terawatts, enough to drive several antimatter factories at full power and produce a gram of antimatter each day. Forward saw the antimatter problem as a matter of scaling and cost (and he often talked about 'small problems of engineering'). As we've seen in the last few days, James Bickford (Draper Laboratory) is more than aware of both these issues, but unlike Forward, he's keen on mining naturally occurring sources of antimatter right here in the Solar System. Forward's huge factories may some day be built, but for now, let's talk about how to get our early antimatter missions into the realm of possibility by...
Finding Antimatter in the Solar System
James Bickford's antimatter work for NASA's Institute for Advanced Concepts, a Phase II study completed just as NIAC was announcing its closure, prompted a number of comments from readers when I opened discussion of it on Monday. And I can see why. We're used to thinking of antimatter production as an extraordinarily expensive process happening only in particle accelerators. And even when we commit the resources to make it, we get only the tiniest amounts, and at costs so high that they make propulsion concepts for antimatter seem chimerical. But Bickford wants us to consider a naturally occurring source of antimatter, one that might offer the potential of being collected in space for a variety of missions. Key to the idea is the fact that high-energy galactic cosmic rays (GCR) continually bombard the upper atmosphere of the planets in our Solar System, as well as interacting with material in the interstellar medium. The result is 'pair production,' the creation of an elementary...
New Discovery Around 55 Cancri
I want to get back to James Bickford's antimatter study tomorrow, at which time I'll set up the full report for download here. This work has already elicited plenty of response, both in comments and backchannel, so tomorrow we'll talk about the mechanisms that create antimatter in our Solar System naturally (as opposed to what we do with particle accelerators), and also ponder how realistic missions to harvest such antimatter could be built around technologies currently in the pipeline. Right now, though, the news conference on 55 Cancri is ongoing, the news from this system more and more interesting now that another planet, the fifth, has been discovered. This is the first system found with this many planets, although the assumption is there will be many, many others. But 55 Cancri, some 41 light years away in the constellation Cancer, bears some resemblances to our own Solar System. The farthest planet from the star is a gas giant about four times Jupiter's mass orbiting every 14...
Antimatter For Deep Space Propulsion
Great ideas fan out in unexpected directions, which is why James Bickford now looks at antimatter in a new light. Bickford (Draper Laboratory, Cambridge MA) realized that an adaptation of Robert Bussard's interstellar ramscoop might have its uses in collecting antimatter. The concept grew out of the realization that antimatter sources were available not only near the Earth but farther out in the Solar System, where antiparticles could be collected and used to boost spacecraft initially to speeds of 100 kilometers per second. That's sufficient for interstellar precursor missions outside the heliosphere, including the possibility of getting a payload to the Sun's gravitational focus, where a new kind of space-based astronomy waits to be exploited. Refine the process enough and you start talking about even greater speeds through more efficient antimatter collection, one great benefit being that instead of producing the stuff in Earth-bound particle accelerators, you're actually mining...
‘Missing Mass’ Theory Revised
Has ten percent of the mass of the universe disappeared? Not really, but it's true to say that our assessment of that mass has to be reconsidered, given recent findings on the nature of x-rays emitted from the vast spaces at the heart of galaxy clusters. How we interpret the x-ray data has a great bearing on how we calculate the mass of gases in the galactic clusters, and the mass of the clusters themselves. The story begins in 2002, when a University of Alabama in Huntsville team studying warm, x-ray emitting gas in galactic clusters reported that it had found large amounts of comparatively low-energy x-rays in addition to higher energy 'hard' x-rays. The so-called 'soft' x-ray emitting atoms were assumed to exist at a density of one atom per cubic meter, but their cumulative mass was thought to amount to as much as ten percent of that needed to hold galactic clusters together. But a closer look at data provided by the Chandra X-Ray Observatory, among other instruments, found no...
White Dwarf Merger (and the Implications)
The recent news about an unusual supernova in Hercules some 300 million light years away has a wider significance than might first appear. Supernovae are important for more than their role in seeding the cosmos with heavy metals forged in their stellar furnaces. They're also widely used cosmological markers. Type Ia supernovae, thought to be well understood, typically occur in a band of brightness that makes them 'standard candles,' useful in calculating cosmic distances. It was work on Type Ia supernovae, in fact, that led to the discovery of the universe's accelerating expansion. And what the latest find implies is that, contrary to earlier thinking, this kind of supernova may be more varied than previously thought. The new find -- supernova 2006gz -- appears to result from the collision of two white dwarfs that had been in orbit around each other. The evidence: a strong spectral signature of unburned carbon and clear signs of compressed layers of silicon. Both spectral signatures...
A Tunguska Reminder
Universe Today offers up the latest edition of the Carnival of Space while announcing it will become the new venue for this gathering of Web links on space-related subjects. Among the posts garnered this time, it's Universe Today's own take on the Tunguska event that should most resonate with Centauri Dreams readers. Tadeusz J. Jopek (Astronomical Observatory UAM in Poland) and team have run simulations of the 1908 explosion to estimate the velocity and impact angle of the Tunguska meteorite. "We believe that TCB originated as the result of a breakup of a single body: a comet or an asteroid. In our study we concluded that it is more probable that it was an asteroid. We cannot point to which one; instead we have found several candidates for the Tunguska parent, and the asteroid 2000 WK63 is an example of it," Dr. Tadeusz said. Interesting! The relevant question, of course, is just how often we can expect such impacts to occur. Tunguska was, happily, a largely unsettled place at the...
A Volcanic Cause of Dinosaur Extinctions?
The Chicxulub crater in the Yucatan gets plenty of press whenever the subject of asteroid deflection comes up, it being the supposed evidence of the 'dinosaur killer' that changed life on Earth forever some 65 million years ago. But other factors may have played a role in the dinosaur extinctions, among them geological events in India, now studied in the form of the so-called 'Deccan Traps,' immense lava beds that show the ancient flow of lava from the same era over an area of hundreds of miles. If current work is correct, the main phase of these eruptions released ten times the amount of climate-altering gases into the atmosphere as Chicxulub itself, which would have occurred more or less at the same point in geological history. And if iridium deposits were an early clue to what happened in the Yucatan, marine sediments and microscopic marine fossils point to the power of the volcanoes. The life forms that created these fossils are known to have evolved just after the extinction...
Reconsidering Gliese 581
Gliese 581 continues to occupy the attention, and understandably so. At least three planets orbit this M-dwarf, one of which sprang into the public consciousness with the announcement that it might be in its star's habitable zone. But both Gl 581c and d are interesting from the habitability standpoint, even if subsequent discussions have pointed out just how problematic it is to make such judgments on insufficient data. Ponder how tricky the call can be. For being in a circumstellar habitable zone only means that a terrestrial-size planet can have liquid water on its surface. A new paper by Franck Selsis (Centre de Recherche Astrophysique de Lyon), James Kasting (Pennsylvania State) and colleagues wades right into this morass, pointing out how many other factors could make such a planet remain uninhabitable: Water may not be available A high impact rate may prevent the emergence of life The thus far unknown minimum ingredients for life's formation may not be present Gravity may be...
A Closer Look at Vesta
It seems extraordinary to speak of picking up pieces of an asteroid on the surface of the Earth, but the meteorites known as eucrites are confidently identified with Vesta, the brightest asteroid in the sky (and the only one visible with the naked eye). With the Dawn mission on its way to both Ceres and Vesta, we'll learn much more about the composition of both, but Vesta is coming into its own as a most unusual object that has contributed much to the surrounding system. For the 330-mile wide asteroid sports a huge gouge taken out of its south pole, apparently the result of a collision between protoplanetary objects. The hole, some eight miles deep, once contained a half million cubic miles of asteroid material that was subsequently blasted into interplanetary space, where interaction with Jupiter came into play. Gravitational tugging changes orbits, and some of these objects were put onto trajectories that brought them to Earth. Image: A 3-D computer model of the asteroid Vesta...
Hot Jupiters Co-existing with Earth-like Worlds?
One of the surprises of the early planet-hunting era has been the discovery of 'hot Jupiters,' giant planets orbiting extremely close to their parent star. That these planets should be prolific in our catalog at present makes sense given the nature (and limitations) of radial velocity detection methods, but before we started finding them, there seemed little reason to believe gas giants would exist at orbits within 0.1 AU. Now we see them as evidence that protoplanets can migrate during the formation period, probably causing havoc as they pass through the inner system. Are hot Jupiters the bane of terrestrial planets? You would think so, given the above scenario, with a gas giant clearing planet-forming materials out of the inner disk during its passage. But Martyn Fogg and Richard Nelson (University of London) think otherwise. Their new paper looks at models of terrestrial planet formation and finds that inner disks survive the passage of the inbound giant, resuming their planetary...
Notes & Queries 10/27/07
More notes on the 'wandering planet' scenario advanced by John Debes (Carnegie Institution of Washington) and Steinn Sigurðsson (Penn State), which suggests that planets ejected from their stars as their solar systems formed could conceivably keep enough internal heat to maintain an atmosphere and sustain a liquid ocean under ice. Debes' simulations show that a planet with a large moon could survive the ejection process. Noting that between four and five percent of the simulations the duo ran on an Earth-mass planet with Luna-like companion resulted in the 'Earth-Moon system surviving, Debes had this to say in an article in Sky & Telescope: "Anytime something happens in astronomy a few percent of the time, it is interesting to us because on the grand scale of things, it means it's happening a lot and people should probably know about it." Interesting indeed, because a large moon means tidal energies between moon and planet that could cause the interior of the planet to warm. Debes...